Tracking the Footprints of the Radio Pulsar B1727-47: Proper Motion, Host Supernova Remnant, and the Glitches | |
Shternin, P.1; Kirichenko, A.1,2; Zyuzin, D.1; Yu, M.3; Danilenko, A.1; Voronkov, M.4; Shibanov, Yu.1 | |
刊名 | ASTROPHYSICAL JOURNAL |
2019-06-01 | |
卷号 | 877期号:2页码:15 |
关键词 | ISM: individual objects (RCW 114) ISM: supernova remnants pulsars: general pulsars: individual (PSR J1731-4744) |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ab1905 |
英文摘要 | The bright radio pulsar B1727-47, with a characteristic age of 80 kyr, was among the first pulsars discovered 50 yr ago. Using regular timing observations and its interferometric positions at three epochs, we measured, for the first time, the pulsar proper motion of 151 +/- 19 mas yr(-1). At the dispersion measure distance of greater than or similar to 2.7 kpc, this would suggest a record transverse velocity of the pulsar of greater than or similar to 1900 km s(-1). However, a backward extrapolation of the pulsar track to its birth epoch points remarkably close to the center of the evolved nearby supernova remnant RCW 114, which suggests genuine association of the two objects. In this case, the pulsar is substantially closer (similar to 0.6 kpc) and younger (similar to 50 kyr), and its velocity (similar to 400 km s(-1)) is compatible with the observed pulsar velocity distribution. We also identified two new glitches of the pulsar. We discuss implications of our results for the properties of the pulsar and the remnant. |
资助项目 | Australian Government |
WOS关键词 | CORE-COLLAPSE SUPERNOVAE ; TIMING OBSERVATIONS ; FILAMENTARY NEBULA ; NEUTRON-STARS ; PACKAGE ; SIMULATIONS ; DYNAMICS ; PERIODS ; TEMPO2 ; SINGLE |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000469433800014 |
资助机构 | Australian Government ; Australian Government ; Australian Government ; Australian Government ; Australian Government ; Australian Government ; Australian Government ; Australian Government |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/26457] |
专题 | 中国科学院国家天文台 |
通讯作者 | Shternin, P. |
作者单位 | 1.Ioffe Inst, Politekhnicheskaya 26, St Petersburg 194021, Russia 2.Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 877, Ensenada 22800, Baja California, Mexico 3.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China 4.CSIRO Astron & Space Sci, POB 76, Epping, NSW 1710, Australia |
推荐引用方式 GB/T 7714 | Shternin, P.,Kirichenko, A.,Zyuzin, D.,et al. Tracking the Footprints of the Radio Pulsar B1727-47: Proper Motion, Host Supernova Remnant, and the Glitches[J]. ASTROPHYSICAL JOURNAL,2019,877(2):15. |
APA | Shternin, P..,Kirichenko, A..,Zyuzin, D..,Yu, M..,Danilenko, A..,...&Shibanov, Yu..(2019).Tracking the Footprints of the Radio Pulsar B1727-47: Proper Motion, Host Supernova Remnant, and the Glitches.ASTROPHYSICAL JOURNAL,877(2),15. |
MLA | Shternin, P.,et al."Tracking the Footprints of the Radio Pulsar B1727-47: Proper Motion, Host Supernova Remnant, and the Glitches".ASTROPHYSICAL JOURNAL 877.2(2019):15. |
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